Gamma Cephei
(Binary)- 35 Cep
- Gl 903
- Gliese 903
- HR 8974
- BD +76°928
- HD 222404
- GCTP 5725.00
- SAO 10818
- FK5 893
- HIC 116727
- HIP 116727
- IRAS 23372+7721
- 2MASS J23392083+7737563
- TIC 367912480
- TYC 4606-3584-1
- Gaia EDR3 2281778105594488192
Gamma Cephei is a binary star system approximately located 45 light years from our Sun, consisting of a subgiant and a red dwarf star. There is at least one known exoplanet within this system.
LOCATION
Discover the celestial coordinates and distances that help us locate and understand this star's position in space.
When looking at celestial coordinates, you'll see three main position types: Right Ascension (RA) measures east-west position like longitude, Declination (Dec) measures north-south position like latitude, and Parallax helps determine a star's distance from Earth. Together, these coordinates help us pinpoint exactly where objects are in our night sky!
BASIC CHARACTERISTICS
Explore the fundamental properties that define this star's physical nature and evolution.
A star's basic characteristics - its mass, size, temperature, age, and luminosity - are all interconnected. These properties determine the star's life cycle and how it appears to us from Earth. Understanding these relationships helps astronomers classify stars and predict their future evolution.
PHOTOMETRY
Understand how bright this star appears from Earth and its true luminosity in space.
Apparent magnitude is how bright a star looks from Earth, while absolute magnitude is its true brightness from a standard distance of 10 parsecs. The lower the number, the brighter the star - and negative numbers mean extremely bright objects!
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